Abstract
We have observed CO emission near very young low mass stars using the Owens Valley Millimeter Interferometer. The data consist of a snapshot visibility survey of 25 IRAS/NH3 cores and full synthesis maps of two cores, L1262 and L1681B. The two sources show spatially compact (radius ≤ 1017 cm) low velocity outflows. Extrapolating from the snapshot survey, at least 64% and up to 100% of the sources have outflows. The momentum flux in the compact outflows is comparable to that powering larger scale low luminosity outflows. The core L1681B contains an unresolved source with velocity extent and emission asymmetries which are consistent with gravitational infall.
Published Version
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